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- W1645884807 abstract "Recent work on the initial-final mass relation for low- and intermediate-mass stars and the mass distrihution of the nuclei of planetary nebulae sets a lower limit on the initial mass of progenitors of PN which is substantially higher than I Me:;. With such a lower limit the theoretical .:stimales of the deathralc of main sequence stars would be consistent with the observ.:d PN birthrate onl~ if the distance scale due 10 Cudworth (1974) were used. A raised lower limit on the progenitor mass also helps explain the low mean distam:es of planetary nebulae from the galactic plane and the paucity of PN in Population II systems." @default.
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- W1645884807 date "1985-01-01" @default.
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- W1645884807 title "On the Consequences of a New Initial-Final Mass Relation for Low and Intermediate Mass Stars and the Birthrate of Planetary Nebulae" @default.
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